Transverse polarization constraint in an angular spectrum
ID: transverse-polarization-constraint-in-an-angular-spectrum
The transverse polarization constraint in an angular spectrum requires each source-free electromagnetic plane wave component to have electric field orthogonal to its wavevector in the algebraic sense:For an isotropic homogeneous medium with constant permittivity, this follows by inserting a Fourier component into . It restricts the vector fields that can accompany a scalar angular spectrum method calculation.[ref]
Interactive Optics by Sander Konijnenberg, Aurèle J.L. Adam and H. Paul Urbach. Scalar Diffraction Optics, Angular Spectrum Method, vector divergence constraint following the propagation equations
With time dependence and , the relation becomesWhen , the longitudinal field is therefore . It is not an arbitrary third scalar image that can be propagated independently of the first two.
For an original propagating angular-spectrum component with , choosing and forces . Polarization along instead gives a purely transverse-to-axis field for this propagation plane. Thus electromagnetic transversality relative to does not require zero field along the laboratory axis.
For an evanescent angular-spectrum component with , the same choice gives . The dot product is not a Hermitian inner product: there is no complex conjugation of in the Fourier-transformed divergence equation. The imaginary longitudinal amplitude represents a phase relationship, not permission to discard the constraint.
At grazing propagation, , division by fails and the original equation must be used. Boundary conditions, material response and the corresponding magnetic field remain necessary to reconstruct a physical solution. In the strongly paraxial approximation, longitudinal components may be small, but that is an approximation derived from the allowed spectrum rather than a replacement for the vector condition.
New to topics? Read the docs here!